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Galaxy Clustering in the Southern Hemisphere

Published online by Cambridge University Press:  12 April 2016

C.A. Collins
C.A. Collins*
Affiliation:
Astrophysics Group, School of Chemical and Physical Sciences, Liverpool John Moores University, Byrom Street, Liverpool L3 3AF

Abstract

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In this paper some of the major results from the COSMOS and APM digitised galaxy surveys are presented. The main motivation behind these catalogues was to study large-scale structure in the universe. We begin by outlining the importance of such studies to cosmology and discussing the early results from the visually compiled galaxy catalogues. The impact of the digitised catalogues is demonstrated by focussing on three key areas of research; the galaxy-galaxy two-point angular correlation function, the cluster-cluster spatial correlation function, and galaxy number counts.

Information

Type
XII. Cosmology
Information
International Astronomical Union Colloquium , Volume 148: The Future Utilisation of Schmidt Telescopes , 1995 , pp. 510 - 521
Copyright
Copyright © Astronomical Society of the Pacific 1995

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